Asteroseismology of the Kepler target KIC 9204718
1 School of Aviation, Girne American University, University Drive, P.O. Box 5, 99428 Karmi Campus, Karaoğlanoğlu, Kyrenia, Turkey
2 College of Graduate Studies, University of South Africa, PO Box 392, Unisa, 0003 Pretoria, South Africa
3 Institute of Astronomy with NAO, Bulgarian Academy of Sciences, blvd. Tsarigradsko chaussee 72, Sofia 1784, Bulgaria
4 Izmir Turk College Planetarium, 8019/21 sok., No: 22, Izmir, Turkey
Published online: 8 September 2017
The high precision data obtained by the Kepler satellite allows us to detect hybrid-type pulsator candidates more accurately than the data obtained by ground–based observations. In this study, we present preliminary results on the new analysis of the Kepler light curve and high-resolution spectroscopic observations of the pulsating Am star KIC 9204718. Our tentative analysis shows that the star has hybrid-type pulsational characteristics.
© The Authors, published by EDP Sciences, 2017
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